Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6735
Full metadata record
DC FieldValueLanguage
dc.contributor.authorTandon, S. N-
dc.contributor.authorGhosh, S. K-
dc.contributor.authorHutchings, J-
dc.contributor.authorStalin, C. S-
dc.contributor.authorSubramaniam, A-
dc.date.accessioned2020-11-10T02:32:31Z-
dc.date.available2020-11-10T02:32:31Z-
dc.date.issued2017-08-
dc.identifier.citationCurrent Science, Vol. 113, No. 4, pp. 583 - 586en_US
dc.identifier.issn0011-3891-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6735-
dc.descriptionOpen Access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0583.pdfen_US
dc.description.abstractThe AstroSat satellite is designed for multiwavelength astronomy for observations covering a spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multiwavelength studies in coordination with the X-ray telescopes on-board AstroSat, UVIT is used to study a large variety of objects with arcsecond-level spatial resolution. During the first year of observations, UVIT has obtained images in many filter bands in the wavelength range 130–300 nm over a field of ~28, which are being used to study a variety of hot stars, nebulae, stellar clusters and galaxies.en_US
dc.language.isoenen_US
dc.publisherCurrent Science Associationen_US
dc.subjectMulti-wavelength astronomyen_US
dc.subjectUltraviolet Imaging Telescopeen_US
dc.subjectX-ray telescopeen_US
dc.titleUltraviolet Imaging Telescope on AstroSaten_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Ultraviolet Imaging Telescope on A.pdf2.69 MBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.